About black holes with nontrapping interior

Physical arguments related with the existence of black hole solutions havin g a nontrapping interior are discussed. Massive scalar fields interacting w ith gravity are considered. Interior asymptotic solutions showing a scalar field approaching a constant value at the horizon are given. It is argued t hat the coupled Einstein-Klein-Gordon equations can be satisfied in the sen se of the generalized functions after removing a particular regularization designed for matching the interior solution with an external Schwarzschild space-time. The scalar field appears as just avoiding the appearance of clo sed trapped surfaces while coming from the exterior region. It also follows that the usual space integral over T-0(0) in the internal region just give s the total proper mass associated to the external Schwarzschild solution, as it should be expected.